Early history of astronomy
... Western Culture today originated in Mesopotamia around 3,000 B.C. – Today 88 constellations are recognized – The brightest stars in a constellation are identified in order of their brightness by the letters of the Greek alphabet – alpha, beta, and so on ...
... Western Culture today originated in Mesopotamia around 3,000 B.C. – Today 88 constellations are recognized – The brightest stars in a constellation are identified in order of their brightness by the letters of the Greek alphabet – alpha, beta, and so on ...
Constellations Jeopardy
... This graph shows the distance from Earth to five of the stars visible in the night sky. This chart best represents the data. ...
... This graph shows the distance from Earth to five of the stars visible in the night sky. This chart best represents the data. ...
The Science behind the Stars ctY Astrophysics by Spencer McClung
... of stars with three helium atoms combining to form a carbon atom. For the most massive stars, this continues until finally iron is formed. Then the weight is so great that the star collapses in on itself and explodes in a supernova, which is how almost every atom heavier than iron is created. That m ...
... of stars with three helium atoms combining to form a carbon atom. For the most massive stars, this continues until finally iron is formed. Then the weight is so great that the star collapses in on itself and explodes in a supernova, which is how almost every atom heavier than iron is created. That m ...
Stellar Evolution: After the Main Sequence
... As a cluster ages, the main sequence is “eaten away” from the upper left as stars of progressively smaller mass evolve into red giants ...
... As a cluster ages, the main sequence is “eaten away” from the upper left as stars of progressively smaller mass evolve into red giants ...
Due Date: Thursday, November 16, 2006
... The most significant difference between a high-mass star and the Sun will be their lifetime! Look at the HR diagram in Figure 11.1. The lifetime of Spica (10 Msun) is only about 10 million years. The lifetime of Achernar (6 Msun) is only 100 million years…so when we really should not expect the Sun ...
... The most significant difference between a high-mass star and the Sun will be their lifetime! Look at the HR diagram in Figure 11.1. The lifetime of Spica (10 Msun) is only about 10 million years. The lifetime of Achernar (6 Msun) is only 100 million years…so when we really should not expect the Sun ...
a. Recognize the physical attributes of stars in the night sky such as
... How are all stars alike? a. They are the same age. b. They are the same size. c. They are the same color. d. They are all balls of hot gases. Answer: d Stars appear as small points of light in the sky because ________________. a. they are so much dimmer than the sun b. they are so much smaller than ...
... How are all stars alike? a. They are the same age. b. They are the same size. c. They are the same color. d. They are all balls of hot gases. Answer: d Stars appear as small points of light in the sky because ________________. a. they are so much dimmer than the sun b. they are so much smaller than ...
UNIT 4 STUDY GUIDE Objectives
... From what regions do comets originate? Which region is further away? What are asteroids and where are they found? What is the difference between a meteoroid, meteor and a meteorite? What is asteroid belt and where is it located? What is a constellation? What characteristics are used to classify star ...
... From what regions do comets originate? Which region is further away? What are asteroids and where are they found? What is the difference between a meteoroid, meteor and a meteorite? What is asteroid belt and where is it located? What is a constellation? What characteristics are used to classify star ...
August Skies
... The source of the Perseid meteor shower is actually debris from the comet SwiftTuttle. Every year, the earth passes through the debris stream left by the comet and the earth's atmosphere incinerates the particles into the glowing embers called meteors or “falling stars”. The shower peaks early after ...
... The source of the Perseid meteor shower is actually debris from the comet SwiftTuttle. Every year, the earth passes through the debris stream left by the comet and the earth's atmosphere incinerates the particles into the glowing embers called meteors or “falling stars”. The shower peaks early after ...
Uniqueness of the Earth, Lebo, 7-30
... two or more stars would make stable planetary orbits impossible. If no star (planet was thrown out of planetary system) there would be no energy source. Must be a G-type star: If hotter, UV would extinguish life: If cooler, would have to be so close that tidal effects of the star on the planet would ...
... two or more stars would make stable planetary orbits impossible. If no star (planet was thrown out of planetary system) there would be no energy source. Must be a G-type star: If hotter, UV would extinguish life: If cooler, would have to be so close that tidal effects of the star on the planet would ...
TU Muscae and the Early-type Overcontact Binaries
... Double-lined spectroscopic binary: spectral lines of both stars are visible. ...
... Double-lined spectroscopic binary: spectral lines of both stars are visible. ...
Uniqueness of the Earth, Lebo, 7-30
... two or more stars would make stable planetary orbits impossible. If no star (planet was thrown out of planetary system) there would be no energy source. Must be a G-type star: If hotter, UV would extinguish life: If cooler, would have to be so close that tidal effects of the star on the planet would ...
... two or more stars would make stable planetary orbits impossible. If no star (planet was thrown out of planetary system) there would be no energy source. Must be a G-type star: If hotter, UV would extinguish life: If cooler, would have to be so close that tidal effects of the star on the planet would ...
Astronomy - Wappingers Central School District
... Here is my powerpoint from last years coaches conference. I will be updating it to reflect the changes in content in this years rules. I’m not sure yet how to test 50 teams at States on the use of DS9 image viewing software, and won’t ...
... Here is my powerpoint from last years coaches conference. I will be updating it to reflect the changes in content in this years rules. I’m not sure yet how to test 50 teams at States on the use of DS9 image viewing software, and won’t ...
stars - allenscience
... The largest stars shed their layers in a massive explosion called a Supernova. The end result is also a planetary nebula. Supernova are so bright that they can outshine an entire galaxy for a period of time. ...
... The largest stars shed their layers in a massive explosion called a Supernova. The end result is also a planetary nebula. Supernova are so bright that they can outshine an entire galaxy for a period of time. ...
2014 Joseph E. Pesce, Ph.D. 1 Astro 113 Final Exam Review 1. What
... 2. What are the basic stages in the Sun's history? 3. What are the various astronomical distance measures? 4. Suppose the Hubble constant, H = 60 (km/sec)/Mpc. A Certain galaxy is known to ...
... 2. What are the basic stages in the Sun's history? 3. What are the various astronomical distance measures? 4. Suppose the Hubble constant, H = 60 (km/sec)/Mpc. A Certain galaxy is known to ...
Red Dwarfs and Barnard`s star. Their origin and significance to
... A red dwarf is a small and relatively cool star on the main sequence, being a M spectral type. Red dwarfs range in mass from a low of 0.075 solar masses (M☉) to about 0.50 M☉ and have a surface temperature of less than 4000 K. Our sun has 1 solar mass (M☉) and a surface temperature of 6000 K Red dwa ...
... A red dwarf is a small and relatively cool star on the main sequence, being a M spectral type. Red dwarfs range in mass from a low of 0.075 solar masses (M☉) to about 0.50 M☉ and have a surface temperature of less than 4000 K. Our sun has 1 solar mass (M☉) and a surface temperature of 6000 K Red dwa ...
How Is a Star`s Color Related to Its Temperature? - d
... Rigel is blue, and Betelgeuse is red. Capella and our sun are yellow. In this activity you will make your own HertzsprungRussell diagram. You will see how star brightness, color, temperature, and class are related. ...
... Rigel is blue, and Betelgeuse is red. Capella and our sun are yellow. In this activity you will make your own HertzsprungRussell diagram. You will see how star brightness, color, temperature, and class are related. ...
Slide 1
... The naked eye, upon optimum conditions, can see down to around the sixth magnitude, that is +6. Under Pogson's system, a few of the brighter stars now have negative magnitudes. For example, Sirius is –1.5. The lower the magnitude number, the brighter the object. The full moon has a magnitude of abou ...
... The naked eye, upon optimum conditions, can see down to around the sixth magnitude, that is +6. Under Pogson's system, a few of the brighter stars now have negative magnitudes. For example, Sirius is –1.5. The lower the magnitude number, the brighter the object. The full moon has a magnitude of abou ...
Level 6 Stars and Constellations
... much easier to speak of a star in Orion than to give its geometrical position in the sky. There are 88 recognized constellations. ...
... much easier to speak of a star in Orion than to give its geometrical position in the sky. There are 88 recognized constellations. ...
Lecture Note
... • The apparent displacement of a nearby object against a distant fixed background from two different viewpoints. ...
... • The apparent displacement of a nearby object against a distant fixed background from two different viewpoints. ...
15.3 The Lives of Stars
... have dissipated (spreads out) • Size of earth, with same mass as our sun • Turns into a black dwarf when fuel runs out • Neutron Stars • Left over from a supernova ...
... have dissipated (spreads out) • Size of earth, with same mass as our sun • Turns into a black dwarf when fuel runs out • Neutron Stars • Left over from a supernova ...
Astronomy of the Northern Sky—
... The Northern Sky faces mostly away from the Milky Way center. Much of the easy-to-find nebulosity is not in this part of the sky, but there are a few we can detect with naked eye, binoculars or small telescopes, preferably the wide-field or rich-field type. All we can use in the northern sky are in ...
... The Northern Sky faces mostly away from the Milky Way center. Much of the easy-to-find nebulosity is not in this part of the sky, but there are a few we can detect with naked eye, binoculars or small telescopes, preferably the wide-field or rich-field type. All we can use in the northern sky are in ...
the lab handout here
... How does the temperature and luminosity of the Sun compare to that of the other stars on the Main Sequence? ________________________________________________________ ...
... How does the temperature and luminosity of the Sun compare to that of the other stars on the Main Sequence? ________________________________________________________ ...
Perseus (constellation)
Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.